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19962007
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astro-ph2007

Influence of the magnetic field on the thermal condensation

P. Hennebelle, T. Passot

The neutral atomic interstellar medium (HI) is well known to be strongly magnetized. Since HI is a 2-phase medium the questions arise of what is the effect of the magnetic field on…

astro-ph2002

Magnetic Pressure-Density Correlation in Compressible MHD Turbulence

Thierry Passot, Enrique Vazquez-Semadeni

We discuss magnetic pressure and density fluctuations in strongly turbulent isothermal MHD flows in "1+2/3" dimensions. We first consider "simple" nonlinear MHD waves, which allow…

astro-ph2002

Thermal Instability and Magnetic Pressure in the Turbulent ISM

Enrique Vazquez-Semadeni, Adriana Gazol, Thierry Passot +1

We review recent results on the nonlinear development of thermal instability in the context of the turbulent atomic interstellar medium (ISM). First, we pre- sent a brief summary o…

astro-ph2000

The Density Probability Distribution Function in Turbulent, Isothermal, Magnetized Flows in Slab Geometry

Enrique Vazquez-Semadeni, Thierry Passot

We investigate the behavior of the magnetic pressure, , in fully turbulent MHD flows in ``1+2/3'' dimensions by means of its effect on the probability density function (PDF) o…

astro-ph1999

Compressible MHD Turbulence: Implications for Molecular Cloud and Star Formation

E. Vazquez-Semadeni, E. C. Ostriker, T. Passot +2

We review recent results from numerical simulations and related models of MHD turbulence in the interstellar medium (ISM) and in molecular clouds. We discuss the implications of tu…

astro-ph1996

MHD Turbulence, Cloud Formation and Star Formation in the ISM

E. Vazquez-Semadeni, T. Passot, A. Pouquet

We discuss the role of turbulence in cloud and star formation, as observed in numerical simulations of the interstellar medium. Turbulent compression at the interfaces of colliding…